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The Spin Tensor of Dark Matter and the Hubble Parameter Tension
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abstract
Allowing for a nonvanishing spin tensor for cold dark matter ($\omega_{\mathrm{DM}}=0$) has the consequence of giving rise to an effective $\mathrm{FLRW}$ dynamics with a small negative barotropic constant for an effective dark matter density ($-1/3<\omega_{\mathrm{eff}}\leq0$). This turns out to solve the Hubble parameter tension in a straightforward way.
Forward citations
Cited by 1 Pith paper
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No late-time role for adiabatic torsion: a no-go result for Hubble-cutoff holographic dark energy in Einstein--Cartan cosmology
The adiabatic Einstein–Cartan torsion mode cannot rescue Hubble-cutoff holographic dark energy: it is dynamically inert and bounded to Ω_Φ < 5×10⁻²⁴ by BBN.
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